RMS Images are meant to represent the root-mean-square deviation from the mean (rmsd) appropriate to measure the noise level in a Gaussian distribution.

maximum 8.4009e-04 Jy/beam
minimum 1.2240e-04 Jy/beam
mean 2.3227e-04 Jy/beam
median 1.7690e-04 Jy/beam
sigma 1.1688e-04 Jy/beam
MAD rms 4.9553e-05 Jy/beam

RMS images

TSKY0001.sb32503898.eb32530404.57613.06443417824_split.ms

Pilot.ql.SgrA_e3.J180740_253000.10.2048.v1.I.iter1.image.pbcor.tt0.rms.sky.png

No pipeline QA for this task.
vis
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SgrA_e3.J180740-253000_P33330v1_2019_01_18T00_17_20.687/working/TSKY0001.sb32503898.eb32530404.57613.06443417824_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SgrA_e3.J180740-253000_P33330v1_2019_01_18T00_17_20.687/working
Start time
2019-01-18 14:40:17.232
End
2019-01-18 14:41:20.853
Duration
0:01:03.621
Note, WebLog generation is not included in the time.

CASA logs for stage 6